Search for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors
- NázevTitle
- Search for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectorsSearch for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors
- Druh výsledkuResult type
- Článek v časopiseJournal article
- AutořiAuthors
- S. Aiello, A. Albert, M. Alshamsi, S. Alves Garre, Z. Bardačová, E. Eckerová, F. Mamedov, Y. Shitov, I. Štekl
- Klíčová slovaKeywords
- gamma ray bursts theory, neutrino astronomy, neutrino experiments
- ExperimentCollaboration
- KM3NeT
- DOIDOI
- 10.1088/1475-7516/2024/08/006
- Časopis / citaceJournal / citation
- Journal of Cosmology and Astroparticle Physics 2024(08), 006 (2024) · ISSN 1475-7516
- RokYear
- 2024
- JazykLanguage
- eng
- ZáznamyRecords
- ProjektProject
- Hodnocení radioaktivity materiálu a vylepšené kalibrační techniky pro zvýšení výkonnosti neutrinových teleskopů KM3NETMaterial radioactivity evaluations and improved calibration techniques to advance performances of the KM3NET neutrino telescopes
- CitovánoCited by
- 23 (INSPIRE-HEP)
- Plný text (open access)Full text (open access)
- https://iopscience.iop.org/article/10.1088/1475-7516/2024/08/006/pdf
- Citace ke staženíDownload citation
- TXT · BibTeX
AbstraktAbstract
Gamma-ray bursts are promising candidate sources of high-energy astrophysical neutrinos. The recent GRB 221009A event, identified as the brightest gamma-ray burst ever detected, provides a unique opportunity to investigate hadronic emissions involving neutrinos. The KM3NeT undersea neutrino detectors participated in the worldwide follow-up effort triggered by the event, searching for neutrino events. In this paper, we summarize subsequent searches, in a wide energy range from MeV up to a few PeVs. No neutrino events are found in any of the searches performed. Upper limits on the neutrino emission associated with GRB 221009A are computed.
Gamma-ray bursts are promising candidate sources of high-energy astrophysical neutrinos. The recent GRB 221009A event, identified as the brightest gamma-ray burst ever detected, provides a unique opportunity to investigate hadronic emissions involving neutrinos. The KM3NeT undersea neutrino detectors participated in the worldwide follow-up effort triggered by the event, searching for neutrino events. In this paper, we summarize subsequent searches, in a wide energy range from MeV up to a few PeVs. No neutrino events are found in any of the searches performed. Upper limits on the neutrino emission associated with GRB 221009A are computed.